Bifurcation theory

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Name (Hebrew)
תורת ההסתעפות
Name (Latin)
Bifurcation theory
Name (Arabic)
نظرية التشعب
See Also From tracing topical name
Differential equations, Nonlinear Numerical solutions
Stability
MARC
MARC
Other Identifiers
Wikidata: Q1154357
Library of congress: sh 85013940
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Wikipedia description:

Bifurcation theory is the mathematical study of changes in the qualitative or topological structure of a given family of curves, such as the integral curves of a family of vector fields, and the solutions of a family of differential equations. Most commonly applied to the mathematical study of dynamical systems, a bifurcation occurs when a small smooth change made to the parameter values (the bifurcation parameters) of a system causes a sudden 'qualitative' or topological change in its behavior. Bifurcations occur in both continuous systems (described by ordinary, delay or partial differential equations) and discrete systems (described by maps). The name "bifurcation" was first introduced by Henri Poincaré in 1885 in the first paper in mathematics showing such a behavior.

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